Articles | Volume 36, issue 3
https://doi.org/10.5194/angeo-36-891-2018
https://doi.org/10.5194/angeo-36-891-2018
Regular paper
 | 
20 Jun 2018
Regular paper |  | 20 Jun 2018

Differentiating diffuse auroras based on phenomenology

Eric Grono and Eric Donovan

Viewed

Total article views: 3,005 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,985 958 62 3,005 72 64
  • HTML: 1,985
  • PDF: 958
  • XML: 62
  • Total: 3,005
  • BibTeX: 72
  • EndNote: 64
Views and downloads (calculated since 06 Mar 2018)
Cumulative views and downloads (calculated since 06 Mar 2018)

Viewed (geographical distribution)

Total article views: 3,005 (including HTML, PDF, and XML) Thereof 2,840 with geography defined and 165 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 14 Dec 2024
Download
Short summary
The solar wind reshapes Earth's magnetic field to create our magnetosphere and powers many dynamic processes in our plasma-filled environment, some of which produce the aurora. Networks of ground-based all-sky cameras are valuable tools that offer a large field-of-view with which to study the aurora. Using sequences of auroral images, this study defines criteria for differentiating an important type of aurora whose subcategories are often conflated.